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HAL Id: jpa-00246869

https://hal.archives-ouvertes.fr/jpa-00246869

Submitted on 1 Jan 1993

HAL is a multi-disciplinary open access archive for the deposit and dissemination of sci- entific research documents, whether they are pub- lished or not. The documents may come from teaching and research institutions in France or abroad, or from public or private research centers.

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upon graphite

A. Rakotomahevitra, C. Demangeat, J. Parlebas, G. Moraitis, E.

Razafindrakoto

To cite this version:

A. Rakotomahevitra, C. Demangeat, J. Parlebas, G. Moraitis, E. Razafindrakoto. Electronic structure

model for single B, C or N adatoms upon graphite. Journal de Physique I, EDP Sciences, 1993, 3

(11), pp.2299-2309. �10.1051/jp1:1993246�. �jpa-00246869�

(2)

Classification

Physics

Abstracts

71.55-73.20

Electronic structure model for single B, C

or

N adatoms upon

graphite

A-

Rakotomahevitra(~),

C.

Demangeat(~),

J-C-

Parlebas(~),

G.

Moraitis(~)

and E.

Razafindrakoto(~)

(~)

I-P-C-M-S--G-E-M-M-E-

(UM

46

CNRS),

Universit4 Louis Pasteur, 67070

Strasbourg,

France

(~) Ddpartement

de

Physique,

Universitd Marien

Ngouabi, Brazzaville, Congo (~)

Laboratoire

d'Energdtique,

BP 906,

Ankatso,

Antananarivo,

Madagascar

(Received

17

February

1993, revised 11 June 1993, accepted 20

July1993)

Abstract. An extra-orbital

tight-binding

scheme and a

repulsive Born-Mayer

model are

used to determine the total

adsorption

energy of a

2p

adatom

(B,

C or

N)

at the surface of

graphite.

The

corresponding

electronic structure of the adsorbed atom is deduced for the most

stable

(hollow) position.

Our model allows us to exhibit an increase of the local

density

of states on the adatom and a decrease of

charge

transfer

(from

adatom to

carbon)

when

going

from boron to

nitrogen.

1 Introduction.

Nitrogen

adsorbed upon

graphite

is one of the

adsorption systems

for which various exper- imental and theoretical results exist

[1-5]-

Also

graphite

is one of the most

commonly

used materials in

atomic-force-microscopy (AFM)

[6] and

scanning-tunnelling-microscopy

[7] studies of surface

morphology. Recently

progress has been achieved in

molecular-dynamics

simulations of the metallic

tip-substrate

interaction in AFM

[8].

Also the interaction

energies

between a

sharp

Pd

tip

with one apex atom and

graphite

were studied on the basis of

first-principle

cal- culations

[9, 10].

Moreover there is a

general

interest in the

study

of the electronic structure of transition metal adatoms upon

graphite

since

graphite

is an ideal substrate for such

adsorbates;

for

example

open

questions

are the conditions of appearance of local

magnetic

moments at V adatoms

[11]

or also the

general

electronic structure trends

along

the 3d series of adatoms.

Because carbon

occupies

a middle

position

in the order of

electronegativity

of the elements in the

periodic table, graphite

welcomes many chemicals

(especially 2p

or

3d)

as adsorbates.

In the

present

paper we restrict our

study

to the electronic structure of

light 2p

atoms

(B, C, N)

adsorbed upon

graphite,

at the

beginning

of

adsorption,

I-e- when isolated adatoms pre-

dominate. More

precisely

we focus our attention on one

(sixfold)

hollow adsorbed atom and we

(3)

develop

a

simple

extra-orbital

tight-binding (EOTB)

model. The

simplicity

of the model based

on electron

sharing

between adsorbate and

substrate,

as well as its self-consistent

screening

in

the sense of Friedel

[12], permits

us to describe the trends in

chemisorption properties

of the

adatoms

along

the

2p

series. It is also

interesting

from an electronic

point

of view to com-

pare the

present adsorption-situation

to

previously

considered

single-impurity

intercalation- situation in bulk

graphite [13-15].

As for an

adatom,

a total energy

calculation, taking

into account both band structure and

repulsive contributions,

is able to

provide

the most stable

position

of the adsorbed

atom,

in a

given geometrical position,

hollow for

example

in the

present

work. The actual adsorbate

position

is

usually

assumed to be the site with the

largest

coordination number

(here six)

available on the surface. This paper is

organized

as follows:

in section 2 we first calculate the band structure of a

basal-plane

surface of

graphite

within

the

tight-binding (TB)

method as well as the

corresponding

intersite Green functions. Next

we

present

our EOTB

adsorption

model

(Sect. 3)

and our method to find out the most stable

(hollow) position

upon

graphite

from a total energy

computation (Sect. 4)- Finally (Sect. 5)

we exhibit and discuss our numerical results for

B, C,

N adatoms.

2. Band structure of a

graphite

surface.

Recently

the

interlayer

interactions within a

bilayer

of

graphite

have been studied

using

local

density approximation [16].

It

happens

that the

interlayer

distance is

only

0.7 To

larger

in

a

bilayer

than in the bulk

graphite;

also the intercarbon distance within a

graphite layer

is

practically

the same for a

bilayer

and for bulk

graphite.

In the

present study

we assume that

graphite

surface is well

represented by

a

bilayer

of

graphite

within TB method. In this method the

parameters corresponding

to1r and a bands

[13]

are fitted

[17].

The

bilayer

is obtained

by disregarding

the further

hopping integrals

n~2 and n~5 in a

bulk-graphite

model

[18].

In our

band structure calculation we use the

following hybridized sp~

atomic

orbitals, (lR), (2R), (3R)

built from linear combinations of

(sR), (xR), (yR)

and the

nonhybridized (4R)

orbital

just given by:

14fl)

=

lzfl) (1)

Then,

the

density

of states

(DOS)

per

spin

at a carbon site R is

given

in terms of the

bilayer graphite

Green function

G°(E)

ni(E)

=

-(1/7r) ~

Im

Gti(E); Gti(E)

=

iii (E+ H°)

-~

ti) (2)

In

equation (2)

t

=

I,

A and H° is the

bilayer graphite

Hamiltonian. In order to determine the electronic structure of an adatom

(next section)

we also need to define and calculate intersite Green functions as

[14]:

G(~(, (E)

=

(tR( (E+ H°)~~ ji'R') (3)

In our numerical

application

we consider 10 000

k-points

in the reduced Brillouin zone

[15], keeping,

the

k-components parallel

to the

bilayer.

Our results for the carbon DOS of a

graphite bilayer

is in fair

agreement

with reference

[16].

It is

interesting

to

decompose

the carbon DOS

(Fig. I)

into

(I)

air,contribution

(arising

from

(4R) orbitals)

which is

unique

in the

vicinity

(4)

E

~

E

j

I

l

~

2 o pi

ul

O

C

-20

ENERGY

(eV )

Fig.

1- Density of states

(DOS)

of

a bilayer of

graphite: x(- -)

and

a(-)

contributions.

of the Fermi level

(EF

= -0.05

eV),

and

(it)

a a-contribution which is also

unique

at

higher energies.

At intermediate

energies

both a and1r

symmetries

contribute.

3. Electronic

adsorption

model.

The EOTB Hamiltonian for an adatom A on

graphite

is then written as H

=+ the

following

terms:

~ 'lll~) ~i (lll~'

+

~ ('lll~) fli~

(i~~~' ~

~.C.)

~

~ '~~)

~~~R

(~)

(i~~~'

(~)

m Rtm Rt

in

equation (4), Et

is the energy level introduced

by

the adsorbed orbital

(mA)

at site A at a distance h

abovilthe graphite

surface with the atomic orbital

symmetry

m = s, x, y, z for adatoms

belonging

to the

2p series; flf(

is the

hopping integral

between the adsorbed atomic orbital

(mA)

and a

surrounding

carbon molecular orbital

(tR) (t

=

1, 4)

it is

expressed

in terms of Slater-Koster atomic

hopping integrals [19].

In the last term of

equation (4)

V(t~ (A) designates

the additional

perturbation potential

at carbon site R due to the

adsorption phenomenon.

From a numerical

point

of view

(see

Sect.

5) Et

and

V(t~ (A)

will be determined for a

given

h from:

(i)

the Friedel sum rule which is

expressed

in terms of

Gh(E),

the

perturbed

Green function associated to H

2

Zh (EF)

"

Ni> (5)

Zh

jE)

=

-11 /7r)Im /~

lY

(Gh iE') G°(E')) dE' (6)

(5)

with

N(

=

3, 4,

5

corresponding respectively

to the number of external s and p electrons

brought by

A

=

B, C, N,

and with

Zh(E) defining

the total number of

displayed

states per

spin,

up to the energy

E,

after the

adsorption

of an A atom at a distance h above the

graphite

surface.

ii)

the local

neutrality

on the cluster

AC6

when A

occupies

a hollow

position

upon a carbon

hexagon

of

graphite:

E~ 6

2

/ fifA(E)

+

~j 6fifR(E)

dE

=

N( (7)

R=1

In

equations (5)

and

(7)

the factor 2 stands for the

spin degeneracy

and the local DOS

(LD OS)

per

spin

at site A is defined

by:

fifA(E)

=

(-1/1r)Im ~j Gii(E), (8)

whereas the variation of the LDOS at a carbon site R due to the

adsorption

is:

~M~(E)

=

(-i/~r)

im

~ (Gj~(E) Gjj(E)) (g)

i

Actually

within a first order

expansion

in terms of

V(~~ (A),

it is

quite

easy to

explicit

the

perturbed

Green functions of

equation (8):

it is a

straightforward

extension of

equations (2.2), (2.3)

and

(2A)

in reference

[15].

A similar

expression

has been derived for

6fifR(E)

in equa-

tion

(9) [20].

4. Total

adsorption

energy.

There is an

interesting point

in the

adsorption problem:

the exact

height

h of the adatom A above the

graphite

surface is determined

through

a total energy calculation

corresponding

to the

adsorption

process of atom A. The

general

definition

[21]

of the total

adsorption

energy

Ead(h)

of an A atom at a distance h above

graphite

is

given by

a sum of

(I)

an attractive

(band

contribution) Ebs(h)

term,

(it)

an electronic Coulomb term

Eee(h)

which has to be subtracted because it has been counted twice in

Ebs(h)

and

(iii)

a

repulsive (Born-Mayer contribution) Er(h)

term:

Ea~(h)

=

E~~(h) E~~(h)

+

E~(h) (io)

The band structure term can be written as follows with an evident notation:

Ebs(h)

= E

(A/graphite)

E

(A) E(graphite) (11)

After a bit of

manipulation, Ebs

can be cast into the

following

form:

Ebs(h)

= 2

EF Zh (EF)

2

/

~~

Zh(E)

dE

~j N(~EQ (12)

~

where

N(~

is the electron number of

symmetry

m

brought by

the adatom A and

Em

is the

corresponding

atomic level. The electronic Coulomb term is

given by

the

following expression

(6)

[22, 23]:

Eee(h)

=

~j U( bN((h) N(~

+

~bN((h) (13)

in

~

bNl(h)

"

Nl(h) Nl~

~ "

IA> Rj

n

=

js, pj (14)

where

bN((h)

is the variation of the local electron number at site I and of

symmetry

n due to the

adsorption,

whereas

N((h)

is the local electron number after

adsorption

of A within a distance h. Also

U(

is the intrasite Coulomb energy between two n electrons at site I. The

repulsive

term

Er(h)

can be

phenomenologically represented by

a

Born-Mayer potential:

it describes at short distances the ion,ion

repulsive

interaction between the A atom and the

neighbouring

carbon atoms of the

graphite

surface. The

general phenomenological

form of

Er

is written as follows

[24]

in terms of the

height

h of the adatom above

graphite:

Er(h)

= a

exp(-a h) (15)

where a and a are the parameters of the

Born-Mayer potential

which characterize each

type

of

adsorption.

For

example

in the case of an adsorbed carbon atom upon

graphite

a

= 208 eV

and a

= 3.3

(I)~~ according

to reference

[25].

For

simplicity

and due to a lack of

data,

in the

following section,

we will

keep

the above carbon

parameters

also for boron and

nitrogen adatoms,

since these elements are close

by

in the classification table. Of course the

equilibrium position ho

of the adatom

corresponds

to the energy minimum of

Ead(h)

as we will see in the next section.

5. Numerical results and discussion.

The

hopping integrals (flf() appearing

in

equation (4)

are calculated

according

to references

spa, ppa and

pplr [19]. We also scaled

the

ntegrals in rder

to be

able to

in pure graphite [20].

The

ifference of energy levels

E[

- E[ (see Eq. (4))

which characterizes

the adatom

A is

taken from lementi [26]. The

value

U[ (= U[) for

nitrogen is

2.39 eV cording to reference [21]. The rresponding values for

boronand arbon

are

educed

from that

for

itrogen,proportionally

to

the

atomic

values [27]. The ratio of the corresponding

perturbation potentials ((A)/V((A)

(see Eq.

(4) with V(~~ (A)

e

V((A) on a eighbouring

graphite site) is

ssumed

to be

given

by the

ratio

of

the

rystal

field

calculated

similarly to the opping ntegrals. Finally

we

end up with two unknown variables

E[

and

V((A)

: they

are

self-consistently determinedthroughequations (5) and (7) as explained

in

section

.

This

is

true

for

a given

eight h

of

A

right

toms. The last step of our

omputation is

to find

out the ost

stable

height

to

a minimum of

the

total

adsorption

energy.

To do this the zero of energy

is assumed

to

level. Next the graphite

band

is ocated so as to satisfy theexperimental ork function

value for graphite [28]

;

in

this case the

Fermilevel

is

at

-5

eV. Then

Em of

equation (12)

also taken from

Clementi [26]. Figure 2 our results of

the

total

adsorption

energy for B, C and N datoms.

The

ost stable heights ho are

0.85 I

and

1.06 I (see

also Fig. 3a) which

correspond to distances

between

the adatom and

the aphite carbon neighbours f1.74

I,

1.65

I and

1.77

I

(Notice that the

C-C

8hortest

distance

within

a xagon in aphite is 1.42

I whereas in

the ntercalation

(7)

(

a

) BORON

1.02 A

o.80

( b ) CARBON

Ms

>

aJ 0.85 A

_

~_ O.80 DO 20

~j

©~

$ 2~

~Z~

(

c

) NITROGEN

I-OS A

o.8a 1-no

Distance above

graphite surface (Al

Fig- 2- Total

adsorption

energy for a boron

(a), carbon(b)

or

nitrogen (c)

adatom

(hollow position)

with respect to its distance above

graphite

surface.

of Refs.

[14, 15]

the two first carbon

neighbours

of an interstitial atom are at 1.83

I

and the

four next nearest at 2.09

I).

Moreover the

charge

transfer from A toward the

graphite

carbon

neighbours

is

decreasing along B,

C and N

(Fig. 3b).

This

suggests

a

change

in

chemisorption

from a rather

strong coupling

situation in the case of boron to a rather weak

coupling

situation

(8)

(a )

~

~

.

i

,'

#

~i

p6

~o "

B

(bj

t O

"~

#

~ ,

2 ',

[

O ,

i~ '.~

fl ~~

~J

B c N

Adsorbate

Fig.

3. -Distance above

graphite (a)

and

charge

transfer ratio

MG/N(

from the adatom to the

graphite

carbon atoms

(b)

with respect to the considered adsorbate

(B,

C,

N).

in the case of

nitrogen.

For the most stable hollow

positions,

it is

interesting

to exhibit the

corresponding

LDOS for

boron,

carbon and

nitrogen

adatoms

(Fig. 4).

In all three cases as in the intercalation case

[15],

there is a

strong

virtual bound state

(vbs)

at the Fermi

level,

the

origin

of which is

essentially 2p~

and

2py

note that these two contributions are not

strictly

identical from

symmetry

reasons between x and y within a

hexagon

of carbon atoms. However since the difference between x and y is

small,

we exhibit x + y on one hand and z in the other

(Fig. 5).

The vbs at

EF

is less filled for boron

(Fig. 4a)

and rather filled for

nitrogen (Fig. 4c).

Also in the three cases of

figure

4 due to a

corresponding strong

adsorbate-substrate

hopping integral

there is an extended s bound state below the

graphite

band

[20]

the

filling

of which

increases from boron to

nitrogen.

Our main numerical results are summarized in table I.

In this paper we have studied the most stable

(hollow) position

of a

2p light

adatom

(B, C, N)

upon

graphite

surface

by using

a total

adsorption

energy calculation.

Although

our EOTB

approach

for the band structure contribution is

quite crude,

we are sure to

satisfy

the Friedel

sum rule as well as a local

neutrality

condition on the adatom and its first

graphite

carbon

neighbours.

Our model allows us to exhibit an increase of the local

density

of states on the adatom and a decrease of

charge

transfer

(from

adatom to

carbon)

when

going

from boron to

(9)

a)

E

~/ b )

E CARBON

E

~

~ j

I

~

(

-20

ENERGY (eV

Fig. 4. Local density of states

(LDOi)

of

a boron

(a),

carbon

(b)

and

nitrogen (c)

adatom upon

graphite

at the most stable

(hollow) height.

The Fermi level

(EF

" -0.05

eV)

is visualised

by

a dashed

line. The s bound state below the

graphite

band is

represented by

a thin

straight

line.

nitrogen.

The

pre8ent

calculation will be extended to the case of transition metal adatoms upon

graphite

for which there is a number of

interesting experimental

data. Another

interesting

(10)

(

~

)

z,

BORON

(

~

)

z,

BORON

x+ y

z

~+

>

~ )

z,

CARBON

( h )

z,

CARBON

I '1

x+ y

z

~

~

+4

q/

ill

O

" "

Cl

-J

(

~

)

z,

NITROGEN

(

~

)

z,

NITROGEN

x+ y

z

-20 -lo 0 lo -20 -20 -lo 0 lo -20

ENERGY ( eV

Fig.

5. Contributions of

(p~

+

py)

and pz orbitals to the local

density

of states

(LDOS)

of a boron

(a),

carbon

(b)

and nitrogen

(c)

adatom upon

graihite

at the most stable

(hollow) position.

extension of the

present

model would be to describe the evolution of the electronic

adsorption

of one

given

element when

going

from one

single

adatom

(as

is the case in the present

paper)

to one

single overlayer

with

possible

metallization upon

graphite.

These

investigations

are now

under progress.

(11)

Table I- The most stable

height

ho of adatom

A, corresponding

distance

do (bond length )

to each of the carbon atoms of the considered substrate

hexagon, perturbation potentials Vi

on the six

graphite

carbon

neighbours

of

A,

final

charge MA

upon

A,

final

charge

transfer

MG

onto the six

graphite neighbours

of A after

adsorption, charge N( initially brought by

A with A =

B, C, N,

s energy level introduced

by

the adsorbed

(sA) orbital,

intrasite Coulomb energy

U[

between two p electrons at site A-

A Carbon

ho (I)

1.02 0.85 1.06

do (I)

1.74 1.65 1.77

V((A) (eV)

0.22 0.05 -0-01

MA

" 2

/~~ fifA(E)

dE 1.14 2.69 3.63

MG

= 2

/ f 6fifR(E)

dE 1.86 1.31 1.37

~~~

3.00 4.00 5.00

(eV)

7.60 -4.32 -11.38

U[ (= U[) (eV)

1.42 1.89 2.39

Acknowledgements.

The authors would like to thank the referees for their

pertinent

remarks.

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